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• W2775796914 abstract "The mode-switching pulsar PSR B0943+10 has been extensively studied in the radio band for many years and, more recently, it has been found to vary also in X-rays, with a flux anticorrelated with the radio emission. Here we review the results of long observations of PSR B0943+10 carried out with XMM-Newton and the LOFAR, LWA and Arecibo radio telescopes in 2014. These results support a scenario in which both unpulsed non-thermal emission, likely of magnetospheric origin, and pulsed thermal emission from a small polar cap (∼1500 m2) with a strong non-dipolar magnetic field (∼ 1014 G), are present during both radio modes and vary in intensity in a correlated way." @default.
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• W2775796914 date "2017-12-01" @default.
• W2775796914 modified "2023-09-30" @default.
• W2775796914 title "X-ray properties of the mode-switching pulsar PSR B0943+10" @default.
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• W2775796914 doi "https://doi.org/10.1088/1742-6596/932/1/012009" @default.
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